Spatially Resolved Molecular Hydrogen Emission in the Inner 200 AU Environments of Classical T Tauri Stars

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dc.contributor.authorBeck, Tracy
dc.contributor.authorMcGregor, Peter
dc.contributor.authorTakami, Michihiro
dc.contributor.authorPyo, Tae-Soo
dc.date.accessioned2015-12-08T22:20:02Z
dc.date.issued2008
dc.date.updated2015-12-08T08:27:43Z
dc.description.abstractWe present 2.0-2.4 μm integral field spectroscopy at adaptive optics spatial resolution (∼0.1″) obtained with the Near-infrared Integral Field Spectrograph (NIFS) at Gemini North Observatory of six classical T Tauri stars: T Tau, DG Tau, XZ Tau, HL T
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/31821
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Stars: formation; Stars: individual (DG Tau, HLTau, HV Tau C, RW Aur, T Tau, XZ Tau); Stars: pre-main-sequence; Stars: winds, outflows
dc.titleSpatially Resolved Molecular Hydrogen Emission in the Inner 200 AU Environments of Classical T Tauri Stars
dc.typeJournal article
local.bibliographicCitation.lastpage489
local.bibliographicCitation.startpage472
local.contributor.affiliationBeck, Tracy, Gemini Observatory
local.contributor.affiliationMcGregor, Peter, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationTakami, Michihiro, Subaru Telescope
local.contributor.affiliationPyo, Tae-Soo, Subaru Telescope
local.contributor.authoremailrepository.admin@anu.edu.au
local.contributor.authoruidMcGregor, Peter, u8401248
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4362859xPUB86
local.identifier.citationvolume676
local.identifier.doi10.1086/527528
local.identifier.scopusID2-s2.0-42149108740
local.identifier.thomsonID000254086100035
local.identifier.uidSubmittedByu4362859
local.type.statusPublished Version

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